Skip to content
Surf Wiki
Save to docs
general/amor-asteroids

From Surf Wiki (app.surf) — the open knowledge base

3552 Don Quixote

Eccentric near-Earth asteroid


Eccentric near-Earth asteroid

FieldValue
minorplanetyes
name3552 Don Quixote
background#FFC2E0
image3552Don2-LB4-mag15.jpg
caption
discovery_ref
discovered26 September 1983
discovererP. Wild
discovery_siteZimmerwald Obs.
mpc_name(3552) Don Quixote
alt_names1983 SA
named_afterDon Quixote fictional character
mp_categoryNEOAmor
Mars-crosser
Jupiter-crosser
Centaur
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc33.71 yr (12,312 days)
aphelion7.2783 AU
perihelion1.2399 AU
semimajor4.2591 AU
eccentricity0.7089
period8.79 yr (3,211 days)
mean_anomaly332.47°
mean_motion/ day
inclination31.092°
asc_node350.03°
arg_peri316.42°
moid0.3338 AU
jupiter_moid0.4397 AU
tisserand2.3150
dimensionskm
rotation7.7 h
albedo0.03
spectral_typeD (Tholen)D (SMASS)
abs_magnitude12.9
magnitude11.67 (1957) to 22.32

Mars-crosser Jupiter-crosser Centaur

3552 Don Quixote, provisionally designated , is an exceptionally eccentric asteroid, classified as a near-Earth object of the Amor group, Mars-crosser and Jupiter-crosser, as well as a weakly active comet.

Discovery and naming

The asteroid was discovered on 26 September 1983, by Swiss astronomer Paul Wild at Zimmerwald Observatory near Bern, Switzerland. It was named after the comic knight who is the eponymous hero of Cervantes Spanish novel Don Quixote (1605). The approved naming citation was published by the Minor Planet Center on 2 December 1990 (M.P.C. 17466).

Orbit and characteristics

Don Quixote is characterized as a dark D-type asteroid in the Tholen and SMASS taxonomy.

It has a highly inclined comet-like orbit of 31 degrees that leads to frequent perturbations by Jupiter. Don Quixote measures 18.4 kilometres in diameter and has a rotation period of 7.7 hours.

Due to its comet-like orbit and albedo, Don Quixote has been suspected to be an extinct comet. However, infrared observations with the Spitzer Space Telescope at 4.5 μm revealed a faint coma and tail around the object. The cometary activity is inferred by carbon dioxide () molecular band emission. In March 2018 a tail was observed at visible wavelengths for the first time. The observation of cometary features during two apparitions suggests that cometary activity is recurrent and Don Quixote is most likely a weakly active comet.

Notes

References

References

  1. Mommert, Michael. (March 2018). "CBET 4502: 20180329 : (3552) DON QUIXOTE". Central Bureau of Electronic Telegrams (Harvard).
  2. (1 June 2020). "Recurrent Cometary Activity in Near-Earth Object (3552) Don Quixote". The Planetary Science Journal.
  3. "JPL Close-Approach Data: 3552 Don Quixote (1983 SA)".
  4. "European Asteroid Research Node:(3552) Don Quixote".
Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

Want to explore this topic further?

Ask Mako anything about 3552 Don Quixote — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.

Report